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Joseph P. Anderson

18 papers hereh-index 10511 citations20 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author9
  • last author1

Across the 14 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO9
  • astro-ph.HE8
  • astro-ph.GA1
same name
  • Joseph P. Anderson — 71 papers, h 37
  • Joseph P. Anderson — 13 papers, h 6
  • Joseph P. Anderson — 8 papers, h 2
  • Joseph P. Anderson — 6 papers, h 3
  • Joseph P. Anderson — 4 papers, h 2
  • Joseph P. Anderson — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102026
most citedProgenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation

176 citations · 568 across the 16 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.HE2024★ 4 cited

Unveiling the nature of SN 2022jli: The first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late times

Régis Cartier, Carlos Contreras, Maximilian Stritzinger +6

We present optical and infrared observations from maximum light until around +800 days of supernova (SN) 2022jli, a peculiar stripped-envelope (SE) SN showing two maxima, each one…

astro-ph.HE2024

Discovery and Extensive Follow-Up of SN 2024ggi, a nearby type IIP supernova in NGC 3621

Ting-Wan Chen, Sheng Yang, Shubham Srivastav +45

We present the discovery and early observations of the nearby Type II supernova (SN) 2024ggi in NGC 3621 at 6.64 +/- 0.3 Mpc. The SN was caught 5.8 (+1.9 -2.9) hours after its expl…

astro-ph.HE2024★ 11 cited

The metamorphosis of the Type Ib SN 2019yvr: late-time interaction

Lucía Ferrari, Gastón Folatelli, Hanindyo Kuncarayakti +32

We present observational evidence of late-time interaction between the ejecta of the hydrogen-poor Type Ib supernova (SN) 2019yvr and hydrogen-rich circumstellar material (CSM), si…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.